September 2042 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Monday, September 29, 2042,[1] with an umbral magnitude of −0.0011. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring only about 9 hours before perigee (on September 29, 2042, at 19:45 UTC), the Moon's apparent diameter will be larger.[2]

Earlier sources compute this as a 0.3% partial eclipse lasting under 12 minutes,[3] but newer calculations list it as a penumbral eclipse that never enters the umbral shadow.

Visibility

The eclipse will be completely visible over eastern Australia, northeast Asia, and western North America, seen rising over east Asia and western Australia and setting over eastern North America and South America.[4]

File:Lunar eclipse from moon-2042Sep29.png File:Lunar eclipse chart close-2042Sep29.png

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[5]

September 29, 2042 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.95481
Umbral Magnitude −0.00105
Gamma −1.02617
Sun Right Ascension 12h23m37.3s
Sun Declination -02°33'13.4"
Sun Semi-Diameter 15'57.9"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 00h25m38.7s
Moon Declination +01°38'07.3"
Moon Semi-Diameter 16'42.1"
Moon Equatorial Horizontal Parallax 1°01'18.0"
ΔT 80.7 s

Eclipse season

Script error: No such module "Labelled list hatnote". This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of September–October 2042
September 29
Ascending node (full moon)
October 14
Descending node (new moon)
October 28
Ascending node (full moon)
File:Lunar eclipse chart close-2042Sep29.png File:SE2042Oct14A.png File:Lunar eclipse chart close-2042Oct28.png
Penumbral lunar eclipse
Lunar Saros 118
Annular solar eclipse
Solar Saros 144
Penumbral lunar eclipse
Lunar Saros 156

Related eclipses

Eclipses in 2042

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 118

Inex

Triad

Lunar eclipses of 2042–2045

Template:Lunar eclipse set 2042-2045

Saros 118

Template:Lunar Saros series 118

Tritos series

Template:Lunar Tritos series December 2009

Inex series

Template:Lunar Inex series October 2013

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[6] This lunar eclipse is related to two annular solar eclipses of Solar Saros 125.

September 23, 2033 October 4, 2051
File:SE2033Sep23P.png File:SE2051Oct04P.png

See also

References

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  6. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

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